运载火箭圆柱形贮箱中推进剂大幅晃动的数值模拟

运载火箭飞行过程中,贮箱内推进剂晃动及波面破碎现象会对燃料贮箱产生较大的干扰力,控制不当会影响飞行稳定性.为了研究推进剂大幅晃动对贮箱结构的影响,建立了圆柱形贮箱内液体晃动非线性动力学模型,利用流体体积函数与水平集法解决了大幅晃动过程中产生的破碎波的描述及自由液面的追踪问题,并对三维圆柱形贮箱在多种含液状态下,由俯仰运...     

一种空间自由曲面非接触扫描测量系统的研究

精确测量空间自由曲面的传统方法是采用三坐标测量机的接触测量或简单的非接触测量,这些测量方法存在工作效率低、自动化程度低等缺点。在深入研究上述方法的基础上,提出了一种自由曲面的非接触自动测量方法,介绍了测量系统的构成、曲面边缘的提取、自动扫描方式的规划以及测头跟踪方式等设计要点。     

感应式表面电位探针的研制

本文描述了感应式表面电位探针原理及实验方法;给出了探针在大气和真空中输出信号大小与表面电位、距离、以及感应片面积之间的关系。为探针设计提供了必要的数据。     

燃油初温对两相爆震性能影响的实验研究

为研究燃油初温对两相爆震性能的影响,在24mm内径爆震管中,以30~200℃的不同初温煤油为燃料,氧气为氧化剂,成功进行了10Hz的两相爆震实验。实验发现,随着燃油初温的升高,火焰锋面的稳态传播速度逐渐增大,爆震燃烧的稳定性逐渐提升,两相爆震峰值压力增大,起爆距离缩短。此外对不同燃油初温下的爆震燃烧尾焰观测表明,油温升高后,非稳态排气总压增大,发动机可获取的推力增大。     

基于外辐射源直达波的对消及仿真研究

利用外辐射源（如调频广播、电视、GPS等的发射信号）的无源雷达探测技术一直是国内外研究的热点。在目标检测上,直达波信号的干扰不但对通道的动态范围提出了极高的要求,同时对微弱目标回波的检测构成了限制。文中利用二元阵的方法对直达波的干扰进行抑制,并对其对消性能进行了仿真分析和研究。     

Enhanced wave and finite element method for wave propagation and forced response prediction in periodic piezoelectric structures

As a promising numerical tool of structural dynamics in mid-and high frequencies, the wave and finite element method (WFEM) is receiving increasingly attention and applications. In this paper, an enhanced WFEM has been developed with a reduced model and a new eigenvalue scheme. The reduced model is applicable for structures with piezoelectric shunts or local dampers;the new eigenvalue scheme can mitigate the ill-conditioning when the wave basis is calculated. The enhanced WFEM is applied to a thin-wall structure with periodically distributed piezoelectric mate-rials (PZT). Both free wave characteristics and forced response are analyzed and the influences of the suggested enhancements are presented. It is shown that if the control factors are properly cho-sen, these enhancements can improve the accuracy while accelerating the calculation. Resulting from the complexity of the application, these enhancements are not optional but imperative.     

波动方程差分解法及其对矩形波导双T形接头的分析

对波动方程差分解法进行了研究 ,给出了电场的计算公式 ,将上述方法应用于矩形波导双T形接头的分析 ,得到了与实测相吻合的各端口反射系数值。     

Plasma electron temperature variability in lunar surface potential and in electric field under average solar wind conditions

The Moon is immersed in plasma environment. The most interesting challenge of the lunar plasma– field environment is that it is alternatively dominated by the extended but variable outer atmosphere of the Earth – the magnetosphere – and by the extended but highly variable solar atmosphere – the solar wind. Understanding the plasma environment and its interaction with the lunar surface will be beneficial to both manned and robotic surface exploration activities and to scientific investigations. Presented is a preliminary map of variations of lunar surface electric potential over the day side and night side using probe equations and a discussion on dust dynamics in this E-field structure using the data from Electron Reflectometer in Lunar Prospector spacecraft during 1998–1999. On the day side, potential is around 5 V and on the night side it reaches up to −82 V. On the night side region, only highly energetic electrons can overcome this large negative potential. The variation at electron temperature (T_e) strongly reflects in the surface potential. The potential reaches to a value of −82 V for T_e = 58 eV. Surface charging causes the electrostatic transport of charged dust grains. Dust grain size of 0.1 μm shows a levitation height of 4.92 m on lunar day side, 748 m on terminator region and 3.7 km on the night side. The radius of maximum sized grain to be lofted, R_max, peaks at the terminator region (R_max = 0.83 μm). At the transition region dust levitation is almost absent. This region is most suited for exploration activities as the region is free from hazards caused by lunar dust.     

First observation of upper mesospheric semi annual oscillations using ground based airglow measurements from Indian low latitudes

We summarize two years of Mesosphere Lower Thermosphere Photometer (MLTP) operation of mesospheric OH and O₂ emission monitoring. The deduced mesospheric OH and O₂ temperatures show large variability. Nightly temperature variations over Gadanki (13.5°N, 79.2°E) are dominated by the short period wave features, while tidal amplitudes are relatively small. Our measurements are the first to report a long period seasonal variation at two upper mesospheric altitudes simultaneously over the Indian sector. Our observations reveal the presence of a dominant semi-annual oscillation (∼6 months periodicity) together with a shorter period (∼2.5  months periodicity) oscillation in both OH and O₂ data.     

Concept options for the aerial survey of Titan

Various aerial platforms intended for long endurance survey of the Titan surface are presented. A few novel concepts are introduced, including a heated methane balloon and a balloon with a tethered wind turbine. All the concept options are predicted to have lower scientific payload fractions than the Huygens probe. It is concluded that the selection of the best aerial platform option depends on more accurate mass estimates and a clear decision on whether, or not, in situ surface composition measurements are required in conjunction with aerial remote sensing.